{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:EHI5ZY6RRG5L3ZXKWVPAW4FMM5","short_pith_number":"pith:EHI5ZY6R","schema_version":"1.0","canonical_sha256":"21d1dce3d189babde6eab55e0b70ac6777d75f35249db065745a1707833e7c6a","source":{"kind":"arxiv","id":"astro-ph/9811219","version":1},"attestation_state":"computed","paper":{"title":"Gamma Radiation from PSR B1055-52","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. J. Thompson, et al","submitted_at":"1998-11-13T15:23:50Z","abstract_excerpt":"The telescopes on the Compton Gamma Ray Observatory (CGRO) have observed PSR B1055-52 a number of times between 1991 and 1998. From these data, a more detailed picture of the gamma radiation from this source has been developed, showing several characteristics which distinguish this pulsar: the light curve is complex; there is no detectable unpulsed emission; the energy spectrum is flat, with no evidence of a sharp high-energy cutoff up to >4 GeV. Comparisons of the gamma-ray data with observations at longer wavelengths show that no two of the known gamma-ray pulsars have quite the same charact"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"astro-ph/9811219","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1998-11-13T15:23:50Z","cross_cats_sorted":[],"title_canon_sha256":"6244e317bbbf7fdd42d3b5886741a968c79c58ebf2ebceb2da66f0d9128861ed","abstract_canon_sha256":"37dc0f86b4d1bb663f3d52d500074cb7309a8702d3826660c2d6b9019296cb35"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:07:11.050867Z","signature_b64":"BuMSnh9Yq/hIwsQp6HZ28XVQ4X5ogf2KwKvmkS7XDnk+O3JKUV04B37grd5zFRy890g7F4/lO3JjEi2WDG/1Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"21d1dce3d189babde6eab55e0b70ac6777d75f35249db065745a1707833e7c6a","last_reissued_at":"2026-07-04T16:07:11.050470Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:07:11.050470Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma Radiation from PSR B1055-52","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. J. Thompson, et al","submitted_at":"1998-11-13T15:23:50Z","abstract_excerpt":"The telescopes on the Compton Gamma Ray Observatory (CGRO) have observed PSR B1055-52 a number of times between 1991 and 1998. From these data, a more detailed picture of the gamma radiation from this source has been developed, showing several characteristics which distinguish this pulsar: the light curve is complex; there is no detectable unpulsed emission; the energy spectrum is flat, with no evidence of a sharp high-energy cutoff up to >4 GeV. Comparisons of the gamma-ray data with observations at longer wavelengths show that no two of the known gamma-ray pulsars have quite the same charact"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9811219","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/9811219/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/9811219","created_at":"2026-07-04T16:07:11.050533+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9811219v1","created_at":"2026-07-04T16:07:11.050533+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9811219","created_at":"2026-07-04T16:07:11.050533+00:00"},{"alias_kind":"pith_short_12","alias_value":"EHI5ZY6RRG5L","created_at":"2026-07-04T16:07:11.050533+00:00"},{"alias_kind":"pith_short_16","alias_value":"EHI5ZY6RRG5L3ZXK","created_at":"2026-07-04T16:07:11.050533+00:00"},{"alias_kind":"pith_short_8","alias_value":"EHI5ZY6R","created_at":"2026-07-04T16:07:11.050533+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5","json":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5.json","graph_json":"https://pith.science/api/pith-number/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/graph.json","events_json":"https://pith.science/api/pith-number/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/events.json","paper":"https://pith.science/paper/EHI5ZY6R"},"agent_actions":{"view_html":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5","download_json":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5.json","view_paper":"https://pith.science/paper/EHI5ZY6R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9811219&json=true","fetch_graph":"https://pith.science/api/pith-number/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/graph.json","fetch_events":"https://pith.science/api/pith-number/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/action/storage_attestation","attest_author":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/action/author_attestation","sign_citation":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/action/citation_signature","submit_replication":"https://pith.science/pith/EHI5ZY6RRG5L3ZXKWVPAW4FMM5/action/replication_record"}},"created_at":"2026-07-04T16:07:11.050533+00:00","updated_at":"2026-07-04T16:07:11.050533+00:00"}